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Table 4
Summary of the residual rms (observed minus calculated flux) of the unbinned and binned data.
| Run | Band | σ | β | σsys |
| [mag] | [mag] | |||
|
|
||||
| Aug. 26 | g′ | 0.0025 | 1.41 | 0.0035 |
| Aug. 26 | r′ | 0.0025 | 1.38 | 0.0035 |
| Aug. 26 | i′ | 0.0028 | 1.45 | 0.0041 |
| Aug. 26 | z′ | 0.0028 | 1.49 | 0.0042 |
| Aug. 30 | g′ | 0.0023 | 1.19 | 0.0027 |
| Aug. 30 | r′ | 0.0017 | 1.10 | 0.0019 |
| Aug. 30 | i′ | 0.0025 | 1.23 | 0.0031 |
| Aug. 30 | z′ | 0.0022 | 1.29 | 0.0028 |
| Oct. 08 | g′ | 0.0018 | 1.22 | 0.0022 |
| Oct. 08 | r′ | 0.0018 | 1.17 | 0.0021 |
| Oct. 08 | i′ | 0.0019 | 1.29 | 0.0025 |
| Oct. 08 | z′ | 0.0020 | 1.33 | 0.0027 |
Notes. σ represents the residual scatter over the entire observing time interval on each run; σsys is the rescaled value for the photometric weights, reflecting the presence of red noise.
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